Pages that link to "Item:Q3575105"
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The following pages link to Numerical relativity confronts compact neutron star binaries: a review and status report (Q3575105):
Displaying 11 items.
- Neutron star merger remnants (Q828790) (← links)
- The evolution of binary neutron star post-merger remnants: a review (Q2059405) (← links)
- Methods for relativistic self-gravitating fluids: from binary neutron stars to black hole-disks and magnetized rotating neutron stars (Q2159314) (← links)
- On the well-posedness of relativistic viscous fluids with non-zero vorticity (Q2804973) (← links)
- Universality in the run-up of shock waves to the surface of a star (Q2891616) (← links)
- NUMERICAL TREATMENT OF ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS: A COMPLEX-PLANE STRATEGY (Q3011498) (← links)
- Full 3D numerical relativity simulations of neutron star–boson star collisions with BAM (Q3383566) (← links)
- AN IMPROVED METHOD FOR CONSTRUCTING MODELS OF SELF-GRAVITATING TORI AROUND BLACK HOLES (Q4649660) (← links)
- Next‐to‐next‐to‐leading order post‐Newtonian linear‐in‐spin binary Hamiltonians (Q5300352) (← links)
- Accurate evolutions of inspiralling neutron-star binaries: assessment of the truncation error (Q5321842) (← links)
- Gravitational wave displacement and velocity memory effects (Q6561105) (← links)